Spectrophotometry of an X-ray source near M33

Details Spectrophotometry of an X-ray source near M33 Spectrophotometry of an X-ray source near M33

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...253l..13c&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 253, Feb. 1, 1982, p. L13-L15.

Astronomy and Astrophysics

Astrophysics

9

Astronomical Spectroscopy, Spectrophotometry, Spiral Galaxies, X Ray Sources, Globular Clusters, Image Dissector Tubes, Radial Velocity

Scientific paper

IIDS spectrophotometry of an object identified with the X-ray source near M33 observed by Long et al. (1981) have been obtained. The source has an apparent radial velocity of 10,800 + or - 800 km/sec, an integrated spectral type similar to a late G or early K giant, and an optical image with noticeably elongated isophotes, suggesting that the source is an elliptical galaxy at z = 0.03 rather than a globular cluster.

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